231 citations · 699 across the 7 of their papers we have counts for
6 papers
Deep 3 GHz Number Counts from a P(D) Fluctuation Analysis
T. Vernstrom, Douglas Scott, J. V. Wall +6
Radio source counts constrain galaxy populations and evolution, as well as the global star formation history. However, there is considerable disagreement among the published 1.4-GH…
The sub-mJy radio population of the E-CDFS: optical and infrared counterpart identification
M. Bonzini, V. Mainieri, P. Padovani +9
We study a sample of 883 sources detected in a deep Very Large Array survey at 1.4 GHz in the Extended Chandra Deep Field South. The paper focuses on the identification of their op…
Resolving the Radio Source Background: Deeper Understanding Through Confusion
J. J. Condon, W. D. Cotton, E. B. Fomalont +6
We used the Karl G. Jansky Very Large Array (VLA) to image one primary beam area at 3 GHz with 8 arcsec FWHM resolution and 1.0 microJy/beam rms noise near the pointing center. The…
Deep 1.1 mm-wavelength imaging of the GOODS-South field by AzTEC/ASTE -- II. Redshift distribution and nature of the submillimetre galaxy population
Min S. Yun, K. S. Scott, Yicheng Guo +22
We report the results of the counterpart identification and a detailed analysis of the physical properties of the 48 sources discovered in our deep 1.1mm wavelength imaging survey…
The VLA Survey of the Chandra Deep Field South. V. Evolution and Luminosity Functions of sub-mJy radio sources and the issue of radio emission in radio-quiet AGN
P. Padovani, N. Miller, K. I. Kellermann +3
We present the evolutionary properties and luminosity functions of the radio sources belonging to the Chandra Deep Field South VLA survey, which reaches a flux density limit at 1.4…
The VLA Survey of the Chandra Deep Field South. II. Identification and host galaxy properties of submillijansky sources
V. Mainieri, K. I. Kellermann, E. B. Fomalont +10
We present the optical and infrared identifications of the 266 radio sources detected at 20 cm with the Very Large Array in the Chandra Deep Field South (Kellermann et al. 2008). U…